NIRCam-selected AGN hosts split into a 'bridge' group with moderate-to-low SFRs and a 'branch' group above the SFMS with SFR rising with AGN fraction; both populations show recent transitions between star formation and quiescence.
Extreme jet-triggered star formation in a z = 4.11 luminous radio galaxy
2 Pith papers cite this work. Polarity classification is still indexing.
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Proposes SKA-VLBI observations of high-redshift jetted AGN to constrain SMBH growth, jet properties, and early-universe cosmology.
citing papers explorer
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PEARLS: Two Distinct Populations of AGN Hosts Moving Between Star Formation and Quiescence
NIRCam-selected AGN hosts split into a 'bridge' group with moderate-to-low SFRs and a 'branch' group above the SFMS with SFR rising with AGN fraction; both populations show recent transitions between star formation and quiescence.
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SKA$-$VLBI view of AGN jets in the early Universe
Proposes SKA-VLBI observations of high-redshift jetted AGN to constrain SMBH growth, jet properties, and early-universe cosmology.